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Generation of magnetic fields by large-scale vortices in rotating convection

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Figure

Figure 1:(color online) Parameter values in (Ek, Ra) parameter space for previous studies�of convective planar dynamos.For compressible convection: K¨apyl¨a et al
Figure 3:(color online) Kinetic (Eu) and magnetic (Eb) energies as a function of Pm. Thedots indicate the mean values, the black vertical lines the range of variation of the energies inthe saturated phase
Figure 4:(color online) Horizontal cross-sections of the axial vorticity at± z = 0.25 for (a)Pm = 0, (b) Pm = 2.5, and (c) Pm = 0.2 at tmax and (d) tmin
Figure 5: (color online) Horizontal power spectra of (a) the velocity (efield (u) and (b) the magneticeb)

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